17O(p,g)18F
Di Leva et al. 2014
The reaction cross section was measured using both the prompt detection of the emitted γ rays and an activation technique. Measurements were carried out at the Laboratory for Underground Nuclear Astrophysics (Gran Sasso, Italy) where the strongly reduced cosmic-ray-induced background allows for improved sensitivity compared to previous studies.
Link to the paper.
Nuclear reaction rate in the MESA format:
Download “17O_pg_DiLevaA_PRC_2014_MESA” 17O_pg_DiLevaA_PRC_2014_MESA.txt – Downloaded 1168 times – 1.02 KBRapagnani et al. 2025
R-matrix cross section calculations by the LUNA collaboration based on available measurements of the relevant nuclear parameters (energies, widths, strengths of known resonances, interference patterns, etc.), coupled to a Monte Carlo to evaluate the global reaction rate error.
Link to paper.
Download “17Opg18F_ChANUREPS_Rapagnani2025” 17O_pg_Rapagnani2025.txt – Downloaded 13 times – 109.38 KBNuclear reaction rate in the MESA format:
Download “17O_pg_Rapagnani _2025_MESA” 17O_pg_Rapagnani-_2025_MESA.txt – Downloaded 156 times – 1.02 KB